GALEX catches dwarf star superflare

June 2, 2005At 2 p.m. Pacific time on April 24, 2004, NASA's Galaxy Evolution Explorer (GALEX), an ultraviolet (UV) space telescope, was studying galaxies in the constellation Virgo when a faint star in its field of view abruptly brightened by more than 10,000 times.

GALEX astronomer Barry Welsh energetically explains the superflare to journalists at the American Astronomical Society's meeting.

On April 24, 2004, the red dwarf star GJ 3685A erupted the largest ultraviolet flare ever seen while NASA's Galaxy Evolution Explorer' satellite was looking its way. The flare peaked twice, pouring out in total about one million times more energy than a typical flare from our Sun. The flare lasted about 20 minutes. See this and other GALEX curiosities in the movies below.

NASA / JPL-Caltech

"It was really more like 20,000 times," says Barry Welsh, a GALEX team member and astronomer at the University of California, Berkeley. "In the far ultraviolet, the flare saturated the detector at 9th magnitude. We're not exactly sure how bright it got," he says. Welsh spoke about the flare at the American Astronomical Society meeting in Minneapolis.

The flaring star is a red dwarf known as GJ 3685A, located about 45 light-years away. The star is 30 percent the size of the Sun and about half as hot, but stars like this comprise 75 percent of those in our galaxy. "At peak flux, the flare was 10 times brighter in the UV than the star itself," Welsh notes.

GALEX picks up large flares from stars every 2 months or so, but they usually result in brightness increases of 100 times. The 2004 superflare was more than 100 times brighter than these  and about a million times more energetic than flares from our own Sun.

"I was surprised by how often we have observed stellar flares and by the amazing size of some of them," says Chris Martin, GALEX's principal investigator. "Nature rarely disappoints us."

GALEX has an unusually large field of view for a space telescope  1.5º  and a detector that actually counts individual photons, measuring both their positions and arrival times to within about a microsecond. "This is very different from a CCD, which just stares and accumulates light," Welsh explains. As a result, the GALEX team recorded the flare in unprecedented detail. "I could show you a movie of the flare with just 0.05 second between frames."

Although designed to study galaxies, GALEX has recorded flare stars, dwarf novae, and pulsating stars, along with asteroids, satellites, and space debris.

"We had no idea the ultraviolet sky would be filled with so many things that go bump in the night," Welsh says, noting that a catalog of flare events will soon be published in The Astronomical Journal. "All of these observations are a bonus to astronomers, since they come free when the telescope is aimed at distant galaxies."

Because GALEX's imager records the arrival times of individual photons, these serendipitous events can be removed cleanly from the spacecraft's all-sky survey. GALEX's mission is to scan the entire sky at ultraviolet wavelengths for clues to how the earliest galaxies evolved into mature galaxies like our own Milky Way.

On April 24, 2004, the red dwarf star GJ 3685A erupted the largest ultraviolet flare ever seen while NASA's Galaxy Evolution Explorer' satellite was looking its way. The flare peaked twice, pouring out in total about one million times more energy than a typical flare from our Sun. The actual flare lasted about 20 minutes. Circular and linear features appearing below and to the right of GJ 3685A are detector artifacts caused by the flare's extreme brightness. NASA/JPL-Caltech

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GALEX spied this probable satellite during the last 5 minutes of a 13.5-minute observation. Faint ghost images on either side of the source are detector artifacts caused by the object's extreme brightness. NASA/JPL-Caltech

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Six mystery objects  most likely space debris near GALEX  fly across the spacecraft's field of view. The two brightest objects seem to perform a sharp turn, then travel in the opposite direction. This apparent motion is a retrograde loop, familiar to astronomers, caused when the spacecraft overtakes the objects as it orbits. NASA/JPL-Caltech